Discussion Overview
The discussion revolves around the concept of proper motion in quasars, exploring whether these distant astronomical objects exhibit measurable motion relative to their surroundings. Participants question the conditions under which quasars might be considered to have proper motion, referencing various articles and studies.
Discussion Character
- Debate/contested
- Exploratory
- Technical explanation
Main Points Raised
- Some participants assert that everything has proper motion, albeit potentially too small to detect for distant objects like quasars.
- Others argue that quasars are so far away that their proper motion is unmeasurably small, leading to their use as fixed reference points in astrometry.
- A participant mentions using Gaia data to search for quasars with zero proper motion, suggesting that most quasars do not exhibit measurable motion.
- There is a discussion about the possibility of measurement errors or misclassification of objects as quasars, with some participants questioning the reliability of the SDSS data.
- Definitions of quasars and their classification as active galactic nuclei are debated, with questions about the distinction between distant and nearby AGNs.
- Some participants bring up the implications of special relativity concerning the velocities of quasars and their redshifts.
- There is mention of specific quasars, such as Markarian 231 and 3C 273, and their classifications, which raises further questions about the criteria for defining quasars versus Seyfert galaxies.
Areas of Agreement / Disagreement
Participants express differing views on whether quasars can have proper motion, with some asserting that they cannot due to their distance, while others suggest that certain quasars may exhibit measurable motion. The discussion remains unresolved, with multiple competing views present.
Contextual Notes
Limitations include the potential for measurement errors, the dependence on definitions of quasars and AGNs, and the unresolved nature of the proper motion measurements discussed.
Who May Find This Useful
Astronomers, astrophysicists, and students interested in the properties of quasars, proper motion in celestial objects, and the classification of active galactic nuclei may find this discussion relevant.